01.03 – Connecting Gravity and Light

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From the course by University of Alberta

Astro 101: Black Holes

4 оценки

University of Alberta

Astro 101: Black Holes

4 оценки

What is a black hole? Do they really exist? How do they form? How are they related to stars? What would happen if you fell into one? How do you see a black hole if they emit no light? What’s the difference between a black hole and a really dark star? Could a particle accelerator create a black hole? Can a black hole also be a worm hole or a time machine? In Astro 101: Black Holes, you will explore the concepts behind black holes. Using the theme of black holes, you will learn the basic ideas of astronomy, relativity, and quantum physics. After completing this course, you will be able to: • Describe the essential properties of black holes. • Explain recent black hole research using plain language and appropriate analogies. • Compare black holes in popular culture to modern physics to distinguish science fact from science fiction. • Describe the application of fundamental physical concepts including gravity, special and general relativity, and quantum mechanics to reported scientific observations. • Recognize different types of stars and distinguish which stars can potentially become black holes. • Differentiate types of black holes and classify each type as observed or theoretical. • Characterize formation theories associated with each type of black hole. • Identify different ways of detecting black holes, and appropriate technologies associated with each detection method. • Summarize the puzzles facing black hole researchers in modern science.

From the lesson

Introduction to Black Holes

Hello and welcome to the first module of Astro 101! In this module, you will become familiar with the basic structure of a black hole, learn the terminology used to describe them, and explore the history of black hole physics.

01.01 – Introduction to Black Holes4:28

01.02 – Black Holes in Pop Culture8:17

01.03 – Connecting Gravity and Light6:38

01.04 – Getting on the Same Wavelength11:01

01.05 – Working with Light15:03

01.06 – Doppler Shift10:23

01.07 – Newtonian Gravity16:29

01.08 – Escape Velocity11:39

01.09 – Dark Stars5:25

01.10 – What is a Black Hole?11:54

01.11 – Black Hole Basics2:39

Meet the Instructors

Sharon Morsink
Associate Professor
Department of Physics, University of Alberta

The relationship between light and

gravity is fundamental to our understanding of black holes.

In order to tie these ideas together,

we will have to relearn the concepts of gravity,

space, time, and light that we've been presented in our favorite movies,

TV shows and other great works of art.

Popular culture doesn't always get the science behind these concepts right.

But it's surprising how scientific accuracy

informs spectacular effects in movies like in Interstellar.

The scientific foundation for black holes has been built

by hundreds of scientists contributing ideas throughout history.

But one unmistakable scientist was responsible for the biggest developments, Einstein.

Einstein's theory of gravity,

describes the gravitational attraction between massive objects,

such as a star or a black hole,

by associating the force of gravity with an equivalent curvature of space,

sort of like this curved sheet.

All physical objects including

rocketships and individual particles of light called photons,

travel on curved space times similar to the curved path that these marbles follow.

In this simple demonstration,

we have an up and down direction defined by the earth's gravity,

which gives us the effect of the marbles orbiting around the central depression.

In outer space, near a star or a black hole,

we don't have earth's gravity holding the marbles down on the curved sheet.

Instead, we recognize gravity as curvature of space and time.

This curved sheet provides valuable insight into how we can

imagine the warping of spacetime.

A black hole is a region of space where the force of gravity becomes so

strong that the curvature of spacetime prevents light from escaping.

In this curved sheet model,

imagine that a marble represents light.

If the marble is aimed away from the center and tossed with a high enough speed,

the marble is able to escape from the depression in the center.

The region outside of a black hole or a normal star is like this,

light that is emitted from objects in

the neighborhood of a black hole are still able to escape.

But there is a special spherical boundary surrounding the black hole,

which scientists call the event horizon.

Once a marble falls within the event horizon,

it must continue falling inwards.

You could try to aim a marble outwards,

but you'd never be able to make the marble go fast enough that it can escape.

To some people, the concept of a black hole is terrifying.

A black hole represents an inescapable vortex,

whose strength can stretch astronauts into spaghetti,

and even eat whole stars.

Falling into a black hole is irreversible,

and once inside, there is no opportunity to escape ever.

To characterize this fear of black holes,

people use the word melanoheliophobia,

the fear of black holes.

Much of that fear is misguided, as you will see,

in black holes come in various flavors that are not equally dangerous.

That's good news if you are among those who suffer from melanoheliophobia, so sit tight.

There is another misconception about black holes that they suck things towards them.

All astrophysical objects like the sun, the earth,

and black holes have gravity,

and gravity is an attractive force.

This means that just as marbles are attracted by gravity to the earth,

so too are they influenced by the gravity of other objects.

If we throw a marble directly towards the earth,

or the sun, or a black hole,

then just like the marble on this curved sheet,

the throne marble traveled directly towards the central depression.

The strength of the gravitational depression

depends on the mass of the object causing it.

A star and a black hole with equal mass,

even though they are different sizes,

produce the same gravitational attraction far from their centers.

If this depression represents a star,

then the stars surface is big and the marble enters the star and is burned up.

Traveling directly towards a star is a recipe for crispy bacon.

Now, let's pretend this depression represents a black hole.

The gravity is exactly the same,

but the black hole is much smaller than the star.

So marbles can travel deeper into the depression before we lose track of it.

When a marble enters the black holes event horizon,

the curvature due to gravity prevents it from escaping and it becomes lost to us forever.

So, even though directly traveling towards a star is a recipe for crispy bacon,

traveling directly towards a black hole is a recipe for no bacon at all.

Instead of traveling directly towards a star or a black hole,

we can instead travel safely around it in orbital paths

similar to how this marble can be made to circle or orbit around the depression.

Since the curve sheet in our demonstration has friction,

the marbles eventually lose energy and fall in towards the center.

However, in space, there is virtually no friction,

so it is possible for orbits to be stable for extremely long periods of time.

For instance, the earth has been orbiting the sun for close to five billion years,

and will continue to orbit it for several billion more years.

The idea that gravity is really just the curvature of spacetime is a tough concept,

which requires some knowledge of Einstein's theory of gravity called general relativity,

which we will be introduced too later on in this course.

However, we can still get a taste of black hole physics by making use of

an older less accurate description of gravity created by Sir Isaac Newton.

In fact, several 18th century physicists were able to deduce the idea of a star,

whose light can't be seen using just their knowledge of

Newton's theory of gravity along with the value for the speed of light.

Since the concepts of light and gravity are so important for understanding black holes,

we will review the basics of

light Newtonian gravity and some elementary physics principles as our starting point.

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